Newborn spheroids at high redshift

When and how did the dominant, old stars in today's massive galaxies form?

S. Kaviraj, S. Cohen, R. S. Ellis, S. Peirani, Rogier Windhorst, R. W. O'Connell, J. Silk, B. C. Whitmore, N. P. Hathi, R. E. Ryan, M. A. Dopita, J. A. Frogel, A. Dekel

Research output: Contribution to journalArticle

32 Citations (Scopus)

Abstract

We study ~330 massive (M* > 109.5M), newborn spheroidal galaxies (SGs) around the epoch of peak star formation (1 < z < 3) to explore the high-redshift origin of SGs and gain insight into when and how the old stellar populations that dominate today's Universe formed. The sample is drawn from the Hubble Space Telescope (HST)/WFC3 Early-Release Science programme, which provides deep 10-filter (0.2-1.7 μm) HST imaging over one-third of the GOODS-South field. We find that the star formation episodes that built our SGs likely peaked in the redshift range 2 < z < 5 (with a median of z ~ 3) and have decay time-scales shorter than ~1.5Gyr. Starburst time-scales and ages show no trend with stellar mass in the range 109.5 < M* < 1010.5 M. However, the time-scales show increased scatter towards lower values (<0.3 Gyr) for M* > 1010.5M, and an age trend becomes evident in this mass regime: SGs with M* > 1011.5M are ~2 Gyr older than their counterparts with M* < 1010.5M. Nevertheless, a smooth downsizing trend with galaxy mass is not observed, and the large scatter in starburst ages indicates that SGs are not a particularly coeval population. Around half of the blue SGs appear not to drive their star formation via major mergers, and those that have experienced a recent major merger show only modest enhancements (~40 per cent) in their specific star formation rates. Our empirical study indicates that processes other than major mergers (e.g. violent disc instability driven by cold streams and/or minor mergers) likely play a dominant role in building SGs, and creating a significant fraction of the old stellar populations that dominate today's Universe.

Original languageEnglish (US)
Pages (from-to)925-934
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume428
Issue number2
DOIs
StatePublished - Jan 2013

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spheroids
merger
galaxies
stars
star formation
trends
star formation rate
universe
time measurement
augmentation
trend

Keywords

  • Cd
  • Galaxies: elliptical and lenticular
  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: high-redshift
  • Galaxies: interactions

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Newborn spheroids at high redshift : When and how did the dominant, old stars in today's massive galaxies form? / Kaviraj, S.; Cohen, S.; Ellis, R. S.; Peirani, S.; Windhorst, Rogier; O'Connell, R. W.; Silk, J.; Whitmore, B. C.; Hathi, N. P.; Ryan, R. E.; Dopita, M. A.; Frogel, J. A.; Dekel, A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 428, No. 2, 01.2013, p. 925-934.

Research output: Contribution to journalArticle

Kaviraj, S, Cohen, S, Ellis, RS, Peirani, S, Windhorst, R, O'Connell, RW, Silk, J, Whitmore, BC, Hathi, NP, Ryan, RE, Dopita, MA, Frogel, JA & Dekel, A 2013, 'Newborn spheroids at high redshift: When and how did the dominant, old stars in today's massive galaxies form?', Monthly Notices of the Royal Astronomical Society, vol. 428, no. 2, pp. 925-934. https://doi.org/10.1093/mnras/sts031
Kaviraj, S. ; Cohen, S. ; Ellis, R. S. ; Peirani, S. ; Windhorst, Rogier ; O'Connell, R. W. ; Silk, J. ; Whitmore, B. C. ; Hathi, N. P. ; Ryan, R. E. ; Dopita, M. A. ; Frogel, J. A. ; Dekel, A. / Newborn spheroids at high redshift : When and how did the dominant, old stars in today's massive galaxies form?. In: Monthly Notices of the Royal Astronomical Society. 2013 ; Vol. 428, No. 2. pp. 925-934.
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